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Impact melt differentiation in the South Pole-Aitken basin: Some observations and speculations
| Content Provider | Semantic Scholar |
|---|---|
| Author | Vaughan, William M. Head, James W. |
| Copyright Year | 2014 |
| Abstract | Abstract The stratigraphy of the South-Pole Aitken basin (SPA) interior is consistent with that of a massive impact melt sheet that differentiated to form cumulates. Spectroscopic and geophysical constraints on the stratigraphy of SPA suggest a ~12.5 km thick layer of norite above ultramafic pyroxenite and dunite layers. A similar stratigraphy is produced from differentiation by crystal settling of a ~50 km thick impact melt sheet (lunar impact melt sheets >10 km thick likely undergo differentiation by crystal settling) formed by an oblique impact (and thus containing ~20 vol. % crustal material). We propose that impact melt differentiation can account for geophysical (nonzero crustal thickness) and geochemical (~2 ppm Th) anomalies in SPA. |
| Starting Page | 101 |
| Ending Page | 106 |
| Page Count | 6 |
| File Format | PDF HTM / HTML |
| DOI | 10.1016/j.pss.2013.11.010 |
| Alternate Webpage(s) | http://www.planetary.brown.edu/pdfs/4543.pdf |
| Alternate Webpage(s) | https://doi.org/10.1016/j.pss.2013.11.010 |
| Volume Number | 91 |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Article |